Erratum:Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits[Chin.Phys.Lett.30(2013) 100402]

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作者
童明雷 [1 ,2 ]
燕保荣 [1 ,3 ]
赵成仕 [1 ,2 ]
尹东山 [1 ,2 ]
赵书红 [1 ,2 ]
杨廷高 [1 ,2 ]
高玉平 [1 ,2 ]
机构
[1] National Time Service Center,Chinese Academy of Sciences
[2] Key Laboratory of Time and Frequency Primary Standards,Chinese Academy of Sciences
[3] Key Laboratory of Precision Navigation and Timing Technology,Chinese Academy of
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  • [1] Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits (vol 30, 100402, 2013)
    Tong Ming-Lei
    Yan Bao-Rong
    Zhao Cheng-Shi
    Yin Dong-Shang
    Zhao Shu-Hong
    Yang Ting-Gao
    Gao Yu-Ping
    CHINESE PHYSICS LETTERS, 2013, 30 (11)
  • [2] Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits
    童明雷
    燕保荣
    赵成仕
    尹东山
    赵书红
    杨廷高
    高玉平
    Chinese Physics Letters, 2013, 30 (10) : 34 - 37
  • [3] Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits
    Tong Ming-Lei
    Yan Bao-Rong
    Zhao Cheng-Shi
    Yin Dong-Shan
    Zhao Shu-Hong
    Yang Ting-Gao
    Gao Yu-Ping
    CHINESE PHYSICS LETTERS, 2013, 30 (10)